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Record W4406766248 · doi:10.3847/1538-4357/ad8eba

Discovery and Spectroscopic Confirmation of Aquarius III: A Low-mass Milky Way Satellite Galaxy

2025· article· en· W4406766248 on OpenAlexfundno aff
W. Cerny, Anirudh Chiti, Marla Geha, Burçı̇n Mutlu-Pakdı̇l, A. Drlica-Wagner, Chin Yi Tan, M. Adamów, Andrew B. Pace, Joshua D. Simon, David J. Sand, Alexander P. Ji, Ting S. Li, A. K. Vivas, Eric F. Bell, Jeffrey L. Carlin, J. A. Carballo-Bello, Astha Chaturvedi, Yumi Choi, Amandine Doliva-Dolinsky, Oleg Y. Gnedin, Guilherme Limberg, C. E. Martínez-Vázquez, S. Mau, G. E. Medina, M. Navabi, Noelia E. D. Noël, Vinicius M. Placco, A. H. Riley, Ian U. Roederer, Guy S. Stringfellow, Clécio R. Bom, P. S. Ferguson, D. J. James, David Martínez‐Delgado, Pol Massana, David L. Nidever, J. D. Sakowska, L. Santana-Silva, Nora Sherman, Erik Tollerud

Bibliographic record

VenueThe Astrophysical Journal · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsnot available
FundersSLAC National Accelerator LaboratoryArgonne National LaboratoryIntegrated Electronics Engineering Center, Binghamton UniversityScience and Technology Facilities CouncilAstrophysics DivisionNatural Sciences and Engineering Research Council of CanadaKavli Institute for Cosmological Physics, University of ChicagoOffice of ScienceUniversity of Illinois at Urbana-ChampaignCentro de Investigaciones Energéticas, Medioambientales y TecnológicasConselho Nacional de Desenvolvimento Científico e TecnológicoChinese Academy of SciencesHigh Energy PhysicsDeutsche ForschungsgemeinschaftLawrence Berkeley National LaboratoryDivision of Astronomical SciencesUniversity of PennsylvaniaFinanciadora de Estudos e ProjetosFundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de JaneiroNuclear Safety and Security CommissionCenter for Cosmology and Astroparticle Physics, Ohio State UniversityUniversity of SussexUniversity of TorontoYale UniversityUniversity of PortsmouthNASA Exoplanet Science InstituteJet Propulsion LaboratoryUniversity of California, Santa CruzOhio State UniversityUniversity College LondonNational Aeronautics and Space AdministrationCalifornia Institute of TechnologyU.S. Department of EnergyW. M. Keck FoundationEuropean Space AgencyFermilabLaboratory Directed Research and DevelopmentNational Science FoundationInstitut de Física d'Altes EnergiesEidgenössische Technische Hochschule ZürichNational Centre for Supercomputing Applications
KeywordsAlgorithmComputer science

Abstract

fetched live from OpenAlex

Abstract We present the discovery of Aquarius III, an ultra-faint Milky Way satellite galaxy identified in the second data release of the DECam Local Volume Exploration survey. Based on deeper follow-up imaging with DECam, we find that Aquarius III is a low-luminosity ( M V = − 2.5 − 0.5 + 0.3 ; L V = 850 − 260 + 380 L ⊙ ), extended ( r 1 / 2 = 41 − 8 + 9 pc) stellar system located in the outer halo (D ⊙ = 85 ± 4 kpc). From medium-resolution Keck/DEIMOS spectroscopy, we identify 11 member stars and measure a mean heliocentric radial velocity of v sys = − 13.1 − 0.9 + 1.0 km s − 1 for the system and place an upper limit of σ v < 3.5 km s−1 (σ v < 1.6 km s−1) on its velocity dispersion at the 95% (68%) credible level. Based on calcium-triplet metallicities of the six brightest red giant members, we find that Aquarius III is very metal-poor ([Fe/H]= − 2.61 ± 0.21) with a statistically significant metallicity spread ( σ [ Fe / H ] = 0.46 − 0.14 + 0.26 dex). We interpret this metallicity spread as strong evidence that the system is a dwarf galaxy as opposed to a star cluster. Combining our velocity measurement with Gaia proper motions, we find that Aquarius III is currently situated near its orbital pericenter in the outer halo (r peri = 78 ± 7 kpc) and that it is plausibly on first infall onto the Milky Way. This orbital history likely precludes significant tidal disruption from the Galactic disk, notably unlike other satellites with comparably low velocity dispersion limits in the literature. Thus, if further velocity measurements confirm that its velocity dispersion is truly below σ v ≲ 2 km s−1, Aquarius III may serve as a useful laboratory for probing galaxy formation physics in low-mass halos.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.003
Threshold uncertainty score0.009

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.000
Science and technology studies0.0010.000
Scholarly communication0.0010.000
Open science0.0000.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0030.001

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.004
GPT teacher head0.210
Teacher spread0.206 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designObservational
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations11
Published2025
Admission routes1
Has abstractyes

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